Classification of candidate Cataclysmic Variables was
accomplished using the 1.5 meter spectrograph at Cerro
Tololo Observatory. Candidate Variables were selected from
the Catalog of Cataclysmic Variables and observed in
low-resolution spectroscopy spanning roughly 6000 angstroms
in the visible and near infrared. Eight objects were
observed and four were classified as Dwarf Novae (Fq Mon, UY
Pup, Oct (LB 9963), and Lib (ASAS 153616-0839.1)). Wy Cma
and Cet (PB 6657) were determined not to be variable and the
two other objects were indeterminable. Funding was provided
by the Cerro Tololo REU program and National Science
Foundation.